具有统计变化的K功率海杂波CA-CFAR调整因子的优化选择

José Raúl Machado Fernández, Jesús de la Concepción Bacallao Vidal
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引用次数: 3

摘要

海杂波干扰信号的存在限制了雷达在沿海和海洋环境中的检测质量。CA-CFAR处理器是检测雷达目标的经典解决方案。它通常在整个运行期间保持其调整系数不变。因此,该方案在执行杂波识别时没有考虑背景信号的缓慢统计变化。为了解决这个问题,作者在MATLAB中对4000万个计算机生成的杂波功率样本进行了密集处理。因此,他们找到了适用于40种可能的杂波统计状态的最佳调整因子值,从而建议使用具有可变调整因子的CA-CFAR架构。此外,还进行了曲线拟合,获得了数学表达式,该表达式概括了整个杂波统计状态范围的结果。用64个细胞的CA-CFAR执行实验,并找到了三种常见误报概率的调整因子值。由于K分布的广泛流行,它被用作杂波模型。本文有助于处理K功率分布,避免使用伽马和贝塞尔函数,这在与K模型相关的开发中很常见。此外,在具有形状参数先验知识的情况下,满足了在K功率杂波中建立自适应杂波检测器的要求。此外,还提出了一些建议,以继续开发更全面的解决方案,该解决方案还将包括形状参数的估计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optimal selection of the CA-CFAR adjustment factor for K power sea clutter with statistical variations
The presence of the sea clutter interfering signal sets limitations on the quality of radar detection in coastal and ocean environments. The CA-CFAR processor is the classic solution for detecting radar targets. It usually operates keeping constant its adjustment factor during the entire operation period. As a consequence, the scheme does not take into account the slow statistical variations of the background signal when performing the clutter discrimination. To solve this problem, the authors conducted an intensive processing of 40 million computer generated clutter power samples in MATLAB. As a result, they found the optimal adjustment factor values to be applied in 40 possible clutter statistical states, suggesting thus the use of the CA-CFAR architecture with a variable adjustment factor. In addition, a curve fitting procedure was performed, obtaining mathematical expressions that generalize the results for the whole addressed range of clutter statistical states. The experiments were executed with a 64 cells CA-CFAR and found the adjustment factor values for three common false alarms probabilities. The K distribution was used as clutter model, thanks to its wide popularity. This paper facilitates the handling of the K power distribution avoiding the use of Gamma and Bessel functions, commonly found in developments related to the K model. Moreover, requirements for building an adaptive clutter detector in K power clutter with a priori knowledge of the shape parameter were fulfill. Also, several recommendations are given to continue the development of a more overall solution which will also include the estimation of the shape parameter.
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